Lambert Azimuthal Equal-Area Projection
The graticule described is for a polar aspect.
Meridians: Equally spaced straight lines intersecting at the central pole. The angles displayed are the true angles between meridians.
Parallels: Unequally spaced circles centered on the central pole. The entire Earth can be shown. Spacing decreases away from the central pole.
Pole: The central pole is a point; the other pole is a bounding circle with 1.41 the radius of the Equator.
Symmetry: About any meridian.
This nonperspective projection is equal-area. Only the center point is free of distortion, but distortion is moderate within 90º of this point. Scale is true only at the center point, increasing tangentially and decreasing radially with distance from the center point. This projection is neither conformal nor equidistant.
There are no standard parallels for azimuthal projections.
This projection was presented by Johann Heinrich Lambert in 1772. It is also known as the Zenithal Equal-Area and the Zenithal Equivalent projection, and the Lorgna projection in its polar aspect.
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